One Ring to Rule Them All ... and in the Darkness Bind Them

By I. Bena, N. Warner. 2004

363 citations recorded by the source corpus.

We construct all eleven-dimensional, three-charge BPS solutions that preserve a fixed, standard set of supersymmetries. Our solutions include all BPS three-charge rotating black holes, black rings, supertubes, as well as arbitrary superpositions of these objects. We find very large families of black rings and supertubes with profiles that follow arbitrary closed curves in the spatial R^4 transverse to the branes. The black rings copiously violate black hole uniqueness. The supertube solutions are completely regular, and generically have small curvature. They also have the same asymptotics as the three-charge black hole; and so they might be mapped to microstates of the D1-D5-p system and used to explain the entropy of this black hole.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/ecd71debbb5cb71da1d7b05d848be1f8940a2e0c

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

In Nuclear and High Energy Physics

Citations in the corpus

Bubbling supertubes and foaming black holes (2005, methodology): “Moreover, in order for the solution to preserve the same supersymmetries as three sets of M2 branes the base space must be hyper-Kähler [13,11,12].”
Black holes, black rings and their microstates (2007, methodology): “Hint 2: You can cheat and use the relation between the charges in the supergravity formula and the integer quantized charges derived in [44] and summarized in (53).”
Black Holes in Higher Dimensions (2008, background): “This was then generalized to a supersymmetric black-ring solution of the U(1)(3) supergravity in [12, 75, 100].”
Supergravity microstates for BPS black holes and black rings (2005, methodology): “Bena and Warner [16] (see also [17]) have developed a formalism for finding five dimensional supersymmetric solutions with three asymptotic charges and two angular momenta as reductions from M-theory.”
Nonsupersymmetric smooth geometries and D1-D5-P bound states (2005, neutral): “Other supersymmetric three-charge solutions have been found in [ 28 , 29, 30], but the regular solutions have not yet been identified or related to CFT states.”
Black Saturn (2007, background): “CTCs tend to appear when solutions are over-spinning, at least that is the case for supersymmetric black holes [36, 31, 32, 33, 15].”
Non-supersymmetric attractors (2005, background): “3), is consistent with the near horizon geometries of the solutions of [55, 56, 57, 58] as discussed in section 5.”
Global structure of five-dimensional fuzzballs (2013, background): “However, yet another miracle happens: the supergravity equations remain linear provided that they are solved in the correct order [26].”
Bicycling black rings (2007, result): “This is similar to the case of supersymmetric black rings [32, 33, 34, 21].”
The fuzzball proposal for black holes (2008, methodology): “Solutions for three charge black holes and black rings have been discussed in [84, 85, 86, 87, 68, 88, 89, 90, 91, 92].”